In General
  > s.a. quantum-gravity phenomenology;
  special relativity [including anisotropy of the speed of light].
  * Motivation for tests:
    An observed violation would be a manifestation of quantum-gravity effects.
  * Possibilities: Small
    shifts of an atom's energy levels, detectable in atomic clocks (&
    Kostelecký); Deviations of cross sections and reaction thresholds
    from standard model predictions (note that Lorentz violation is sometimes
    associated with CPT violation); Modified dispersion relations measurable
    in time-of-flight experiments, including faster than light travel;
    Anisotropies in the speed of light, testable with rotating resonators;
    Vacuum birefringence; Would be associated with a violation of the
    equivalence principle.
  * 2001: In analysis of
    cosmological sources, the coefficients for Lorentz violation are bounded
    by 3 × 1032.
  * 2004: Preferred frame models
    are for all practical purposes ruled out by experimental bounds (& Sudarsky).
  * 2006: Lower bound of 0.0066
    EP ~ 0.66 × 1017
    GeV on violation scale from GRB 051221A; No effect on electron spin down to
    10−21 eV from University of Washington
    torsion-balance experiment [@ news pn(06)apr].
  * 2007: Michelson-Morley
    experiments give bounds of order 10−16
    on coefficients for electrons and photons.
  * 2009: No anisotropy in light
    propagation has been seen at the 10−17 level.
  * 2012: Explicit
    Lorentz-invariance breaking is very tightly constrained by experiment,
    and deformations generically lead to problems with locality.
  * 2014: Michelson-Morley
    experiments give bounds of order 10−18
    on coefficients for electrons and photons.
  * 2015: Tight bound
    >1.6 EP (99% c.l.) for
    energy scale of stochastic fluctuations in photon propagation speed.
  @ General references:
    Amelino-Camelia NJP(04);
    Allen & Yokoo NPPS(04)ht [terrestrial + space based experiments];
    Pospelov & Pomalis PT(04)jul;
    Kostelecký SA(04)sep,
    a0802-conf;
    Mattingly LRR(05)gq;
    Bailey & Kostelecký PRD(06) [framework];
    Liberati PoS-a0706;
    Kostelecký & Russell RMP(11)-a0801-conf [data tables, updated 2010];
    Mattingly a0802-conf [proposals];
    Kostelecký & Mewes ApJ(08)-a0809 [with electromagnetic waves, framework];
    Bluhm a1302-ch [standard model extension, overview];
    Liberati CQG(13)-a1304 [rev];
    Bailey a1505-conf,
    a1906-conf [rev];
    Accioly et al a1604 [photon gravitational deflection].
  > Related topics: see modified
    lorentz group; tests of general relativity with light
    [light bending]; violations of lorentz symmetry.
Earth-Based Tests > s.a. Anisotropy;
  diffraction; Ether [drift].
  @ Interferometry: Lämmerzahl CQG(98)gq;
    Amelino-Camelia & Lämmerzahl CQG(04)gq/03;
    Müller et al PRL(08)
      [Mach-Zehnder atom interferometer and isotropy of gravity];
    Pruttivarasin et al Nat(15)jan-a1412 [Michelson-Morley experiment for electrons];
    Nagel et al nComm(15)-a1412 [precision tests];
    > s.a. Michelson-Morley Experiment.
  @ Gravitational-wave interferometers: Hansen et al PRD(15)-a1412;
    Melissinos a1601-wd;
    Kostelecký & Mewes PLB(16)-a1602;
    Schreck CQG(17)-a1603.
  @ Resonators: Lipa et al PRL(03)
    + pn(03)feb;
    Stanwix et al PRL(05)hp,
    PRD(06)gq [microwave];
    Müller PRD(05);
    Herrmann et al PRL(05),
    PRD(09);
    Müller et al PRL(07);
    Eisele et al PRL(09)
    + news pw(09)sep
      [no isotropy violation at the 10−17 level];
    Baynes et al PRD(11) [non-rotating odd-parity asymmetric optical resonator];
    Michimura et al PRL(13)-a1303 [optical ring cavity].
  @ Hydrogenlike atoms: Belich et al PRD(06)ht;
    Kharlanov & Zhukovsky JMP(07)-a0705;
    de Campos Borges & Barone Rangel EPJC(16)-a1601
      [corrections to the the ground state energy and wave function].
  @ Atomic physics: Bluhm hp/01-conf,
    et al PRL(99),
    et al PRL(02)hp/01 [clocks];
    Russell PS(05) [and optical];
    Hohensee et al PRL(13)-a1303 [dysprosium];
    Pihan-Le Bars et al a1701 [atomic clocks];
    Shaniv et al PRL(18)-a1712;
    Sanner et al a1809 [optical clocks];
    news cosmos(19)mar [atomic clocks].
  @ Bose-Einstein condensates:
    Visser et al ht/01-conf;
    Colladay & McDonald PRD(06);
    Casana & da Silva MPLA(15)-a1106 [ideal bosonic gas].
  @ Beta decay: Noordmans et al PRL(13) [reanalysis of old experiments on forbidden decays];
    Díaz et al PRD(13)-a1305 [bounds on coefficients].
  @ Other experiments:
    Wolf et al PRL(03),
    GRG(04)gq,
    PRD(04)hp [oscillator and maser];
    Kholmetskii PS(03) [Mössbauer spectroscopy];
    Tobar et al PRD(05)hp/04 [photons, scalar + parity-odd coefficients];
    Canè et al PRL(04) [neutrons, bounds on boost effects];
    Cardone et al FP(06) [DC voltage produced by constant B field];
    Kostelecký & Tasson PRL(09)-a0810
    + news ns(09apr [gravity-matter coupling];
    Altschul PRD(10) [electron, boosts],
    PRD(10)-a1005 [electron];
    Bennett et al a1008-conf [tests of gravity];
    DeAngelis et al NCC-a1011-proc [bound on asymmetry of particle lifetimes];
    Noordmans & Vos PRD(14) [charged-pion decay];
    Lo et al PRX(16)-a1412 [using rotating quartz oscillators];
    Abe et Super-Kamiokande PRL(15) [with atmospheric neutrinos, no signs of violations];
    Long & Kostelecký PRD(15)-a1412,
    Kostelecký & Mewes PLB(17)-a1611 [in short-range gravity, tungsten oscillators];
    Shao et al PRL(16)-a1607 [submillimeter scale];
    Kislat & Krawczynski PRD(17)-a1701;
    Tizchang et al EPJC(19)-a1811 [laser beam interacting with charged lepton beam];
    Escobar & Martín-Ruiz PRD(19)-a1902 [ultracold neutrons].
  @ And the equivalence principle:
    Halprin & Kim PLB(99);
    > s.a. classical equivalence principle.
  @ And constants: Kostelecký et al PRD(03)ap/02.
Space-Based and Astrophysical Tests
  > s.a. topological defects.
  * Binary pulsars: Violations of
    Lorentz symmetry in the orbital evolution of binary pulsars would induce a much more
    rapid decay of their orbital periods due to the emission of dipolar radiation.
  @ Space-based: Bluhm et al PRD(03) [and CPT];
    Battat et al PRL(07)-a0710 [lunar laser ranging];
    Klioner et al a1002 [astrometry];
    Overduin et al a1307-conf [constraints from Gravity Probe B];
    Hees et al PRD(15)-a1508 [with planetary orbital dynamics];
    Bourgoin et al PRL(16)-a1607,
    a1706 [lunar laser ranging];
    Pihan-le Bars et al PRL(19)-a1912 [MICROSCOPE space mission].
  @ Using gamma-ray bursts: Rodriguez & Piran JCAP(06)ap,
    et al JCAP(06);
    Xiao & Ma PRD(09)-a0909;
    Maccione et al PRL(10)-a1003 [in stringy spacetime models];
    Stecker APP(11)-a1102 [polarization, absence of birefringence];
    Ellis & Mavromatos APP(13)-a1111 [and AGNs];
    Kostelecký & Mewes PRL(13)-a1301 [improved sensitivity using GRB linear polarization];
    Otte et al a1305-conf [prospects];
    Vasileiou et al PRD(13)-a1305;
    Couturier et al a1308-proc;
    Zhang & Ma APP(14)-a1406;
    Vasileiou et al et al nPhys(15)mar
    + news pw(15)mar [bound on energy scale for photon speed fuzziness];
    Pan et al ApJ(15)-a1505 [Markov chain Monte Carlo approach, no evidence];
    Wei et al ApJ(17)-a1704 [constraints from GRB 160625B];
    Acciari et MAGIC PRL(20) [constraints from GRB 190114C];
    > s.a. gamma-ray astronomy and GRBs;
  phenomenology of lorentz violation.
  @ Very-high-energy photons: Rubtsov et al PRD(14)-a1312 [detection];
    Daniel et al a1508-proc [Cherenkov Telescope Array].
  @ Using neutrinos: Biesiada & Piórkowska JCAP(07)-a0712 [neutrino tof delays];
    Guo et al PRD(12)-a1206 [cmb data and the neutrino sector];
    Amelino-Camelia et al a1307 [using IceCube data];
    Ellis et al a1807 [multimessenger observations of blazar TXS 0506+056].
  @ Using pulsars: Jacobson et al Nat(03)ap/02 [Crab nebula synchrotron radiation];
    Maccione et al JCAP(07)-a0707 [Crab nebula and dispersion relations];
    Altschul PRD(07)hp/06 [neutrons and pulsar timing];
    Xie RAA(13)-a1208 [binary pulsars and constraints on standard model extension];
    Otte a1208-proc [VHE emission from pulsars];
    Shao & Wex CQG(12)-a1209 [small-eccentricity binary pulsars];
    Shao et al a1211-MG13,
    Shao et al CQG(13)-a1307;
    Yagi et al PRL(14)-a1307 [binary pulsars];
    Shao PRL(14)-a1402,
    PRD(14)-a1412 [and standard-model extension];
    Jennings et al PRD(15)-a1510 [binary pulsars].
  @ Using gravitational waves: 
    Sotiriou PRL(18)-a1709 [from black-hole  binaries];
    Mewes PRD(19)-a1905.
  @ Other astrophysics:
    Bailey a0709-conf;
    Biesiada & Piórkowska MNRAS(09)-a0712 [lensing delays];
    Altschul PRD(08) [for pions];
    Jacob & Piran PRD(08)-a0810 [extragalactic gamma-ray sources];
    Tso & Bailey PRD(11) [light bending];
    Boncioli et al a1509-conf [UHE cosmic rays];
    Lorentz & Brun a1606-proc [blazar Mrk 501 flare];
    Bettoni et al JCAP(17)-a1702 [using satellite galaxies];
    Nogués et al PoS-a1710 [combined studies].
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